UDK 53
UDK 520
UDK 521
UDK 523
UDK 524
UDK 52-1
UDK 52-6
GRNTI 41.00
GRNTI 29.35
GRNTI 29.31
GRNTI 29.33
GRNTI 29.27
GRNTI 29.05
OKSO 03.06.01
OKSO 03.05.01
OKSO 03.04.03
BBK 2
BBK 223
TBK 614
TBK 6135
BISAC SCI004000 Astronomy
BISAC SCI005000 Physics / Astrophysics
We determine the selenographic coordinates of the Chandrayaan-3 lander by Doppler measurements of its signal. The Chandrayaan-3 successfully landed in the south polar region of the Moon near the craters Manzinus and Simpelius on 23 August 2023 and had been transmitting scientific information and telemetry to Earth in the S and X-bands during 14 days. The accuracy of the obtained Doppler measurements do not allow unambiguous determination of the lander location on the lunar surface because the transmitter was degrading during the entire observing interval. For this reason, in our work we have evaluated the influence of the Doppler measurement characteristics on the accuracy of the transmitter location determination. It has been shown that for a signal with a relative frequency instability of the order of $10^{-13}$, the achievable accuracy of coordinate determination is about 34 meters.
ephemerides; Moon; space vehicles; techniques: radial velocities; telescopes
1. Brumberg V.A., Glebova N.I., Lukashova M.V., et al., 2004, Transactions of IAA RAS, 10
2. Duev D.A., Molera Calves G., Pogrebenko S.V., et al., 2012, Astronomy & Astrophysics, 541, id. A43
3. Marshalov D., Ping J., Li W., et al., 2020, Latvian Journal of Physics and Technical Sciences, 57, p. 22
4. Murphy T.W. Jr., Adelberger E.G., Battat J.B.R., et al., 2011, Icarus, 211, p. 1103
5. Park R.S., Folkner W.M., Williams J.G., et al., 2021, The Astronomical Journal, 161, id. 105
6. Shuygina N., Ivanov D., Ipatov A., et al., 2019, Geodesy and Geodynamics, 10, 2, p.150
7. Vasilyev M.V., Yagudina E.I., Krasinsky G.A., et al., 2022, Transactions of IAA RAS, 63, p. 28